The Supernova Remnants as the main sources of gamma-quanta with energies more than 1 TeV in our Galactic-Reference-Cited by-同舟云学术

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The Supernova Remnants as the main sources of gamma-quanta with energies more than 1 TeV in our Galactic

Published:2000 Issue: Volume: Page:
ISSN:0094-243X
Container-title:AIP Conference Proceedings
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Author:

Sinitsyna V. G.

Publisher

AIP

Cited by 10 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Cosmic Ray production in SNRs of Pulsar Wind Nebulae type at different ages;EPJ Web of Conferences;2022

2. Shell-type supernova remnants as sources of cosmic rays;Advances in Space Research;2018-11

3. The very high energy characteristics of shell-type SNRs and Pulsar Wind Nebulae at different ages;Journal of Physics: Conference Series;2016-07

4. Long-term observations of the Cyg X-3 and λCygni SNR at ultrahigh energies by SHALON mirror Cherenkov telescopes;Bulletin of the Lebedev Physics Institute;2013-05

5. TeV flaring activity of Cygnus X-3 during 13 years;Nuclear Physics B - Proceedings Supplements;2009-12

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